We present a three-dimensional hot Jupiter model, extending from 200 bar to 1 mbar, using
the Intermediate General Circulation Model from the University of Reading. Our horizontal …

A key legacy of the recently launched the Transiting Exoplanet Survey Satellite (TESS) mission
will be to provide the astronomical community with many of the best transiting exoplanet …

Using a three-dimensional general circulation model, we create dynamical model atmospheres
of a representative transiting giant exoplanet, HD 209458b. We post-process these …

Measurements of the atmospheric carbon (C) and oxygen (O) relative to hydrogen (H) in hot
Jupiters (relative to their host stars) provide insight into their formation location and …

The nearby extrasolar planet GJ 436b—which has been labelled as a ‘hot Neptune’—reveals
itself by the dimming of light as it crosses in front of and behind its parent star as seen from …

There are no planets intermediate in size between Earth and Neptune in our Solar System,
yet these objects are found around a substantial fraction of other stars 1 . Population statistics …

Hot Jupiters, with atmospheric temperatures T≳ 1000 K, have residual thermal ionization
levels sufficient for the interaction of ions with the planetary magnetic field to result in a sizable …

We present a new version of our code for modeling the atmospheric circulation on gaseous
exoplanets, now employing a" double-gray" radiative transfer scheme, which self-…

Remote observing of exoplanetary atmospheres is now possible, offering us access to
circulation regimes unlike any of the familiar solar system cases. Atmospheric circulation models …

Classically derived estimates of heritability from twin models have been plagued by the
possibility of genetic-environmental covariance. Survey questions that attempt to measure …